Araştırma Makalesi
BibTex RIS Kaynak Göster
Yıl 2020, Cilt: 6 Sayı: 2, 98 - 101, 31.07.2020
https://doi.org/10.22399/ijcesen.686962

Öz

Kaynakça

  • [1] Rafelski, Johann and Berndt Muller. Strangeness production in the quark gluon plasma. Physical Review Letters 48 no. 16 (1982): 1066.
  • [2] Markum, H., M. Meinhart, G. Eder, M. Faber, and H. Leeb. "Interactions between quark clusters in lattice QCD." Physical Review D 31, no. 8 (1985): 2029.
  • [3] Pickering, Andrew, and James T. Cushing. "Constructing quarks: A sociological history of particle physics." (1986): 381-383.
  • [4] Griffiths, David. Introduction to elementary particles. John Wiley and Sons 2008.
  • [5] Collins, John C., and Malcolm J. Perry. "Superdense matter: neutrons or asymptotically free quarks?." Physical Review Letters 34, no. 21 (1975): 1353.
  • [6] encyclopedia 2011/11/2 http://en.wikipedia.org/wiki/Equation of state
  • [7] A. Chodos, R. L. Jaffe, K. Johnson, C. B. Thorn and V. F. Weisskopf, Phys. Rev. D 9, 3471 (1974).
  • [8] G. L. Guardo, V. Greco and M. Ruggieri, AIP Conf. Proc. 1595, 224 (2014); [arXiv:1401.7613 [hep-ph]].
  • [9] W. Florkowski, Nucl. Phys. A 853, 173 (2011).
  • [10] Sanches Jr, S. M., F. S. Navarra, and D. A. Fogaça. "The quark gluon plasma equation of state and the expansion of the early Universe." Nuclear Physics A 937 (2015): 1-16.
  • [11] Fogaça, D. A., L. G. Ferreira Filho, and F. S. Navarra. "Nonlinear waves in a quark gluon plasma." Physical Review C 81, no. 5 (2010): 055211.

Thermodynamics of the Quark Gluon Plasma in the Early Universe

Yıl 2020, Cilt: 6 Sayı: 2, 98 - 101, 31.07.2020
https://doi.org/10.22399/ijcesen.686962

Öz

The recent progress in collider experiments provides us with valuable information to understand the properties of the quark-gluon plasma. In this study, we provide the analytical solution to the deferential equation of the time evolution of the temperature in the early Universe in the MIT bag model for gluons only. We discuss the equation of state of a QGP in a particular model, the possible signs for a plasma created in heavy-ion collisions and provide analytic solutions describing the time evolution of the energy density, temperature and pressure of this plasma in the early universe.

Kaynakça

  • [1] Rafelski, Johann and Berndt Muller. Strangeness production in the quark gluon plasma. Physical Review Letters 48 no. 16 (1982): 1066.
  • [2] Markum, H., M. Meinhart, G. Eder, M. Faber, and H. Leeb. "Interactions between quark clusters in lattice QCD." Physical Review D 31, no. 8 (1985): 2029.
  • [3] Pickering, Andrew, and James T. Cushing. "Constructing quarks: A sociological history of particle physics." (1986): 381-383.
  • [4] Griffiths, David. Introduction to elementary particles. John Wiley and Sons 2008.
  • [5] Collins, John C., and Malcolm J. Perry. "Superdense matter: neutrons or asymptotically free quarks?." Physical Review Letters 34, no. 21 (1975): 1353.
  • [6] encyclopedia 2011/11/2 http://en.wikipedia.org/wiki/Equation of state
  • [7] A. Chodos, R. L. Jaffe, K. Johnson, C. B. Thorn and V. F. Weisskopf, Phys. Rev. D 9, 3471 (1974).
  • [8] G. L. Guardo, V. Greco and M. Ruggieri, AIP Conf. Proc. 1595, 224 (2014); [arXiv:1401.7613 [hep-ph]].
  • [9] W. Florkowski, Nucl. Phys. A 853, 173 (2011).
  • [10] Sanches Jr, S. M., F. S. Navarra, and D. A. Fogaça. "The quark gluon plasma equation of state and the expansion of the early Universe." Nuclear Physics A 937 (2015): 1-16.
  • [11] Fogaça, D. A., L. G. Ferreira Filho, and F. S. Navarra. "Nonlinear waves in a quark gluon plasma." Physical Review C 81, no. 5 (2010): 055211.
Toplam 11 adet kaynakça vardır.

Ayrıntılar

Birincil Dil İngilizce
Bölüm Research Articles
Yazarlar

Hamid Al-zakı 0000-0002-1142-8614

Yayımlanma Tarihi 31 Temmuz 2020
Gönderilme Tarihi 9 Şubat 2020
Kabul Tarihi 11 Haziran 2020
Yayımlandığı Sayı Yıl 2020 Cilt: 6 Sayı: 2

Kaynak Göster

APA Al-zakı, H. (2020). Thermodynamics of the Quark Gluon Plasma in the Early Universe. International Journal of Computational and Experimental Science and Engineering, 6(2), 98-101. https://doi.org/10.22399/ijcesen.686962